How is the distance ($d$) to a remote object calculated once its recessional velocity ($v$) is known using Hubble's Law?
Answer
d = v / H_0
By rearranging the expression of Hubble's Law ($v = H_0 d$), the distance ($d$) is found by dividing the measured recessional velocity ($v$) by the Hubble constant ($H_0$).
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